Table 3.
Results of fitting the full FoV spectra of individual pointings expected to show multi-phase substructure.
| Region | C | E | SW |
| kT1 (keV) | 1.30(−0.07, +0.17) | 1.50(−0.09, 0.11) | 1.77(−0.39, 0.08) |
| norm1 | 1.54(−0.34, +0.99) | 2.49(−0.46, +0.54) | 2.33(−1.58, +0.36) |
| v1 (km/s) | −160(−42, +71) | 50(−27, +15) | −152(−198, +27) |
| σv1 (km/s) | 153(−47, +40) | 172(−36, +34) | < 215(2σ u.l.) |
| kT2 (keV) | 1.97(−0.07, +0.17) | 2.44 ± 0.14 | 2.72(−0.47, +0.16) |
| norm2 | 2.91(−1.01, +0.31) | 1.84(−0.55, +0.42) | 1.55(−0.35, +1.29) |
| v2 (km/s) | 18(−12, +29) | −38(−12, +11) | −45(−15, +15) |
| σv2 (km/s) | 151(−25, +14) | < 67(2σ u.l.) | < 97(2σ u.l.) |
| LMXB flux | −11.81(+0.06, −0.05) | −12.44(−0.17, 0.11) | < − 12.56(2σ u.l.) |
| C-stat/d.o.f. | 1922/1970 | 1840/1866 | 3685/3410 |
Notes. All velocities are reported with respect to a rest frame heliocentric redshift of 0.00428. The LMXB flux is given in log(erg/s/cm2) in the 2–7 keV band. The normalizations of the thermal components are given in 1e-2 Xspec units (Eq. (1)).
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